Next: Data Pipeline
Up: ALMA Software Science Requirements:
Previous: Dynamic Scheduling
Subsections
Operator Interface
- Location: The Operator can either be located at the site or at
the Operational Support Facility (OSF) in San Pedro de Atacama.
- Skills: ALMA Operators should have experience with computing
and electronics, with a much higher weighting toward the computing
skills.
The ALMA Operator will be responsible for the smooth operation of the
ALMA by performing the following functions:
- 1.
- Tends to the daily observing schedule, which may involve an
appropriate level of interaction with the dynamic scheduling system.
For example, the Operator should review the observing schedule for his
shift and contact the appropriate staff regarding possible problems
with this schedule.
- 2.
- Ensures overall safety at the site by monitoring work schedules
of engineers and technicians working at the site. For example, if a
telescope is taken out of service for maintenance or repair, the
Operator is the main contact point for information regarding the
progress of this repair work.
- 3.
- Takes care of ``routine'' operational tasks, which may include
the acquisition and analysis of:
- (a)
- baseline determination measurements which follow antenna reconfiguration;
- (b)
- pointing measurements;
- (c)
- flux calibration measurements.
In order to support additional (remote) monitoring of the array
system, the Operator interface software should be made available from
any location. A good operational model for such a system would be any
of the remote monitoring systems available at the existing millimeter
array and single antenna facilities (OVRO, BIMA, NRAO 12 Meter,
PdBI). This interface should include:
- 1.
- a basic ``current array status'' display, which includes
information such as current pointing position for the array (in a
variety of coordinate systems), receiver status, and correlator
configuration;
- 2.
- a weather display indicating the current site conditions;
- 3.
- a video display from cameras at strategic locations on the site
(an extreme would be to place a video camera at each telescope pad
location);
- 4.
- a ``current integration'' display.
Note that the monitor information within this interface
will need to be accessible from everywhere.
Next: Data Pipeline
Up: ALMA Software Science Requirements:
Previous: Dynamic Scheduling
Robert Lucas
2000-05-29